DOE OSTI · 2529500
Higgs Inflation and the Electroweak Gauge Sector
Abstract
Abstract We introduce a method that allows the Higgs to be the inflaton. The Higgs is considered as a pseudo‐Nambu‐Goldstone (pNG) boson of a global coset symmetry , which is spontaneously breaks at an energy scale . A suitable Chern−Simons (CS) interaction is given to it, with representing the dimensionless CS coupling strength and an decay constant. As a result, slow‐roll inflation occurs via ‐induced friction down a steep sinusoidal potential. To obey electroweak symmetry, the lowest‐order CS interaction is required to be quadratic in the Higgs, with the coupling strength . Higher‐order interaction terms keep the full Lagrangian nearly invariant under the approximate pNG shift symmetry. Employing the simplest symmetry coset , ‐folds of inflation occur when . Successfully explaining inflation necessitates small values of the decay constant, ; this in turn requires large , which is ruled out by electric dipole measurements. Although the electroweak hierarchy problem while achieving successful inflation, the real benefit is found in providing a different path to identifying the Higgs as the inflaton, outside the standard modified‐gravity framework.
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Alexander, Stephon [Brown Center for Theoretical Physics, Department of Physics Brown University Providence Rhode Island 02912 USA], Creque‐Sarbinowski, Cyril [Center for Computational Astrophysics Flatiron Institute 162 5th Avenue New York New York 10010 USA], Gilmer, Humberto [Brown Center for Theoretical Physics, Department of Physics Brown University Providence Rhode Island 02912 USA] (ORCID:0000000347129007), Freese, Katherine [Texas Center for Cosmology and Astroparticle Physics Department of Physics The University of Texas at Austin Austin Texas 78712 USA]. 2025-03-01. Higgs Inflation and the Electroweak Gauge Sector. https://doi.org/10.1002/prop.202500020
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